There is a particularly neat way to derive Schrödinger’s equation, and to justify the “canonical substitution” rules for replacing energy and momentum with corresponding operators when we “quantize” an equation.
Take a particle in a potential. Its energy is given by
E=p22m+V(x),
or
E−p22m−V(x)=0.
Now multiply both sides this equation by the formula ei(p⋅x−Et)/ℏ. We note that this exponential expression cannot ever be zero if the part in the exponent that’s in parentheses is real:
[E−p22m−V(x)]ei(p⋅x−Et)/ℏ=0.
So far so good. But now note that
Eei(p⋅x−Et)/ℏ=iℏ∂∂tei(p⋅x−Et)/ℏ,
and similarly,
{\bf p}^2e^{i({\bf p}\cdot{\bf x}-Et)/\hbar}=-\hbar^2{\boldsymbol\nabla}e^{i({\bf p}\cdot{\bf x}-Et)/\hbar}.
This allows us to rewrite the previous equation as
\left[i\hbar\frac{\partial}{\partial t}+\hbar^2\frac{{\boldsymbol\nabla}^2}{2m}-V({\bf x})\right]e^{i({\bf p}\cdot{\bf x}-Et)/\hbar}=0.
Or, writing \Psi=e^{i({\bf p}\cdot{\bf x}-Et)/\hbar} and rearranging:
i\hbar\frac{\partial}{\partial t}\Psi=-\hbar^2\frac{{\boldsymbol\nabla}^2}{2m}\Psi+V({\bf x})\Psi,
which is the good old Schrödinger equation.
The method works for an arbitrary, generic Hamiltonian, too. Given
H({\bf p})=E,
we can write
\left[E-H({\bf p})\right]e^{i({\bf p}\cdot{\bf x}-Et)/\hbar}=0,
which is equivalent to
\left[i\hbar\frac{\partial}{\partial t}-H(-i\hbar{\boldsymbol\nabla})\right]\Psi=0.
So if this equation is identically satisfied for a classical system with Hamiltonian H, what’s the big deal about quantum mechanics? Well… a classical system satisfies E-H({\bf p})=0, where E and {\bf p} are eigenvalues of the differential operators i\hbar\partial/\partial t and -i\hbar{\boldsymbol\nabla}, respectively. Schrödinger’s equation, on the other hand, remains valid in the general case, not just for the eigenvalues.